As shown in Fig. REF , the instrument adopts a modular design and consists of separate visible (\(<\) 940 nm) and infrared (IR, \(>\) 940 nm) benches. This modular design allows concurrent operation of multiple science modules. The IR bench hosts the DM, coronagraphs, and multi-core fiber bundle for REACH (Rigorous Exoplanetary Atmosphere Characterization with High dispersion coronagraphy)[1]} module and sends light to the CHARIS (Coronagraphic High Angular Resolution Imaging Spectrograph)[2]} and GLINT (Guided-Light Interferometric Nulling Technology)[3]} modules, while the visible bench hosts the PyWFS, VAMPIRES (Visible Aperture Masking Polarimetric Imager Resolved Exoplanetary Structures)[4]}, and FIRST (Fibered Imager foR a Single Telescope)[5]} modules. These science modules can be fed with a suite of dichroics and beamsplitters.
